NGC 6404
(Collinder 340; VDBH 240; MWSC 2658; OCL 1024; vdBergh-Hagen 240; ESO 393 13)
0.95
UTI
1.0
CN
1.0
Cdens
1.0
CC3
0.87
Clit
1.0
Cdup
Stellar density (N50/rad)
52.5 [N/pc2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.87 Well-studied
- Cdup 1.0 Unique
Overview
NGC 6404 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the distance, absorption, age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 264.915 | -33.225 | 0.354 | 0.144 | -0.744 | 9.755 |
| Almeida et al. | 2025 | 264.92 | -33.222 | â | â | â | â |
| Hunt & Reffert | 2024 | 264.911 | -33.229 | 0.361 | 0.148 | -0.746 | 59.446 |
| Cavallo et al. | 2024 | 264.912 | -33.22 | 0.361 | â | â | â |
| Hunt & Reffert | 2023 | 264.911 | -33.229 | 0.361 | 0.148 | -0.746 | 59.446 |
| Just et al. | 2023 | 264.906 | -33.234 | â | â | â | â |
| Jaehnig et al. | 2021 | 264.914 | -33.224 | 0.388 | 0.173 | -0.697 | â |
| Rain et al. | 2021 | 264.916 | -33.224 | 0.355 | 0.194 | -0.705 | â |
| Dias et al. | 2021 | 264.92 | -33.222 | 0.357 | 0.198 | -0.698 | 9.38 |
| Cantat-Gaudin et al. | 2020 | 264.916 | -33.224 | 0.355 | 0.194 | -0.705 | â |
| Cantat-Gaudin & Anders | 2020 | 264.916 | -33.224 | 0.355 | 0.194 | -0.705 | â |
| Soubiran et al. | 2018 | 264.916 | -33.224 | â | â | â | 9.91 |
| Bica et al. | 2019 | 264.898 | -33.242 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 264.916 | -33.224 | 0.355 | 0.194 | -0.705 | â |
| Kharchenko et al. | 2016 | 264.906 | -33.234 | â | â | â | â |
| Dias et al. | 2014 | 264.904 | -33.247 | â | -1.01 | -0.59 | â |
| Kharchenko et al. | 2013 | 264.915 | -33.233 | â | 6.3 | -3.37 | 10.6 |
| Morales et al. | 2013 | 264.904 | -33.247 | â | â | â | â |
| Gozha et al. | 2012 | 264.904 | -33.247 | â | â | â | â |
| Ahumada & Lapasset | 2007 | 264.9 | -33.25 | â | â | â | â |
| Dias et al. | 2002 | 264.904 | -33.247 | â | -7.73 | -5.0 | 10.6 |
| Lynga | 1987 | 264.898 | -33.242 | â | â | â | â |
| van den Bergh & Hagen | 1975 | 264.075 | -33.217 | â | â | â | â |
| Sulentic et al. | 1973 | 264.887 | -33.246 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.58 | 3.41 | 2.01 | 500 | 0.110 | 3447 | â | 2 |
| Liu et al. | 2025 | 7.38 | 1.31 | â | 151 | â | â | â | â |
| Almeida et al. | 2025 | 2.77 | 3.65 | â | 6 | â | 3447 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 5852(1) | â | â |
| Cavallo et al. | 2024 | 1.30 | 4.60 | â | 302 | -0.830 | â | â | â |
| Hunt & Reffert | 2023 | 2.64 | 4.39 | 2.01 | 34 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 562 | â | 303 | â | â |
| Jaehnig et al. | 2021 | 2.58(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.60 | 2.90 | â | 501 | â | â | â | 0 |
| Dias et al. | 2021 | 2.77 | 3.65 | â | 6 | 0.285 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.50 | 3.47 | â | 100 | â | â | â | â |
| Kounkel et al. | 2020 | 2.36 | 3.93 | â | 457 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.60 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.60 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.60 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.15 | 3.35 | â | 562 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.15 | 3.35 | â | 562 | 0.110 | â | â | â |
| Morales et al. | 2013 | 2.42 | â | â | 500 | â | â | â | â |
| Gozha et al. | 2012 | 1.70 | â | â | 501 | 0.110 | â | â | â |
| Ahumada & Lapasset | 2007 | â | 2.90 | â | 617 | â | â | â | 5 |
| Dias et al. | 2002 | 2.40 | 2.90 | â | 501 | 0.110 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 151 along with FoF_282.
Palma et al. (2025)
Part of multiple system G77, along with HSC_2946 and LP_282.
Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.92 (50th percentile), true positive (human-assigned).
Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.
Ahumada & Lapasset (2007)
Only straggler candidates inside a radius of 2' around the centre of coordinates have been considered.